Radio frequency interference detection and mitigation for radio astronomy are bottleneck problems. Telescopes are becoming more sensitive therefore thresholds for detecting unwanted signals are becoming lower and telescopes have to deal with a big number of interference sources. When an unwanted signal is detected for radio astronomers it is quite important to know the probability of false alarm Pfa with which signal was detected and to set thresholds with desired Pfa level. LOFAR (LOw Frequency ARray) of radiotelescopes is located in the Netherlands and in other European countries. In the case of LOFAR telescope we look at a detector based on eigenvalue test of covariance matrices. The simple threshold for this test was derived in the work...
Item does not contain fulltextLOFAR is an innovative radio telescope in the frequency range of 10-24...
International audienceRadio astronomical observations are increasingly corrupted by radio frequency ...
This work presents the first RFI detection and mitigation algorithm for the interferometric radiomet...
The next generation of radio telescopes is expected to be one to two orders of magnitude more sensit...
International audienceAims: This paper discusses the spectral occupancy for performing radio astrono...
The Low Frequency Array (LOFAR) is a radio telescope currently being designed. Its targeted observat...
Only a decade after the discovery of radio telescopes astronomers took real interest in this field. ...
In the Northern part of the Netherlands ASTRON is building the largest radio telescope in the world ...
ASTRON is building the world’s largest radio telescope for low frequencies, LOFAR. LOFAR is optimize...
Currently a new low frequency radio telescope is developed in the Netherlands. The telescope is base...
In the North-Western part of Europe, ASTRON is building the world-largest largest low-frequency radi...
Radio astronomical observations are increasingly corrupted by radio frequency interferences. Thus, r...
Radio Frequency Interference (RFI) mitigation is extremely important to take advantage of the vastly...
Item does not contain fulltextLOFAR is an innovative radio telescope in the frequency range of 10-24...
International audienceRadio astronomical observations are increasingly corrupted by radio frequency ...
This work presents the first RFI detection and mitigation algorithm for the interferometric radiomet...
The next generation of radio telescopes is expected to be one to two orders of magnitude more sensit...
International audienceAims: This paper discusses the spectral occupancy for performing radio astrono...
The Low Frequency Array (LOFAR) is a radio telescope currently being designed. Its targeted observat...
Only a decade after the discovery of radio telescopes astronomers took real interest in this field. ...
In the Northern part of the Netherlands ASTRON is building the largest radio telescope in the world ...
ASTRON is building the world’s largest radio telescope for low frequencies, LOFAR. LOFAR is optimize...
Currently a new low frequency radio telescope is developed in the Netherlands. The telescope is base...
In the North-Western part of Europe, ASTRON is building the world-largest largest low-frequency radi...
Radio astronomical observations are increasingly corrupted by radio frequency interferences. Thus, r...
Radio Frequency Interference (RFI) mitigation is extremely important to take advantage of the vastly...
Item does not contain fulltextLOFAR is an innovative radio telescope in the frequency range of 10-24...
International audienceRadio astronomical observations are increasingly corrupted by radio frequency ...
This work presents the first RFI detection and mitigation algorithm for the interferometric radiomet...